33 Polyhymnia
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33 Polyhymnia is a main belt asteroid that was discovered by French astronomer Jean Chacornac on October 28, 1854<ref name="IAU_MPC"/> and named after Polyhymnia, the Greek Muse of sacred hymns.
Rotation
Photometric observations of this asteroid at the Organ Mesa Observatory in Las Cruces, New Mexico during 2008 gave a light curve with a period of 18.609 ± 0.002 hours and a brightness variation of 0.15 ± 0.02 in magnitude. This result is in good agreement with a previous study performed during 1980.<ref name="Pilcher2009"/> These results were re-examined with additional observations in 2011, yielding a refined estimate of 18.608 ± 0.001 hours and a brightness variation of 0.18 ± 0.02 magnitude.<ref name="Pilcher2011"/> In 2020, an analysis of photometric data of Polyhymnia from 2008 to 2019 determined a more precise rotation period of Template:Val. Two possible north pole orientations of Polyhymnia were also determined, with both solutions indicating an axial tilt of 151–155° (ecliptic latitudes –61° to –65°) with respect to the ecliptic.<ref name="Franco2020"/>
Orbit
On its highly eccentric (0.338) orbit around the Sun, 33 Polyhymnia appears brightest (apparent magnitude 10) at its minimum distance from Earth of 0.91 AU.<ref name="AstDyS2014"/> Its orbit puts it in a 22:9 mean-motion resonance with the planet Jupiter. The computed Lyapunov time for this asteroid is 10,000 years, indicating that it occupies a chaotic orbit that will change randomly over time because of gravitational perturbations of the planets.<ref name="Sidlichovsky"/> Measurements of the position for this asteroid from 1854 to 1969 were used to determine the gravitational influence of Jupiter upon 33 Polyhymnia. This yields an inverse mass ratio of Template:Val for Jupiter relative to the Sun.<ref name="Janiczek1970"/>
Mass and density
In 2012, a study by Benoît Carry gave a meta-estimate of a mass of Template:Val for Polyhymnia, based on a single study of its gravitational influence on other Solar System bodies.<ref name="Carry2012"/> However, given Polyhymnia's diameter of Template:Cvt, this mass implies an extremely high density of Template:Val. Such a high density is unrealistic, so this mass and density estimate of Polyhymnia was considered unreliable by Carry.<ref name="Carry2012"/> Several other asteroids with diameters similar to Polyhymnia were also measured to have extremely high densities in Carry's study, and were rejected for being unrealistic.<ref name="Carry2012"/> Because of Polyhymnia's small size, its gravitational influence on other bodies is extremely difficult to detect and may lead to highly inaccurate mass and density estimates.<ref name="Carry2012"/> For example, the Template:Cvt-diameter asteroid 675 Ludmilla was originally measured to have a density of Template:Val in Carry's study,<ref name="Carry2012"/> but improved orbit calculations in 2019 showed that it had a much lower density of Template:Val.<ref name="SiMDA-675"/>
No other peer-reviewed study has attempted to determine a mass and density for Polyhymnia since Carry's study,<ref name="SiMDA-33"/> though in 2023, researcher Fan Li performed a preliminary analysis of Polyhymnia's close approaches with other asteroids and determined a lower mass of Template:Val.<ref name="Li2023-39045"/> Depending on the diameter used for Polyhymnia, this mass estimate suggests a density of Template:Val or Template:Val, for an occultation-derived diameter of Template:Cvt and infrared-derived diameter of Template:Cvt, respectively.<ref name="Li2023-39045"/><ref name="Li2023-39046"/>
Composition
Visible light spectroscopy of Polyhymnia from 1995 and 2002 show that it is an S-type asteroid, meaning it is mainly composed of rocky silicates.<ref name="jpldata"/> In particular, Polyhymnia's spectrum exhibits an absorption band at 0.67 μm wavelengths, which indicates olivine and pyroxene on its surface, similar to Q-type asteroids.<ref name="Bus2002"/>Template:Rp Since Polyhymnia shares both characteristics of S- and Q-type asteroids, it is further classified as an Sq-type asteroid according to the SMASS classification.<ref name="Bus2002"/>Template:Rp Radio telescopes have studied Polyhymnia by radar in 1985.<ref name="detected"/><ref name=baas30_1450/>
In 2023, researchers Evan LaForge, Will Price, and Johann Rafelski speculated the possibility that Polyhymnia could be composed of high-density superheavy elements near atomic number 164, if Polyhymnia's extremely high density were correct and superheavy elements could be sufficiently stable.<ref>Template:Cite journal</ref> However, as noted above, Polyhymnia very likely does not have such a high density.<ref name="Li2023-39045"/><ref name="Li2023-39046"/>
References
External links
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